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Paper Citation Record · LEDGER

A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1810.05181.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1810.05181 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-05-21T02:13:55.459985Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 7c602cf4-84a0-4480-bfa1-f09e20e9b11e · inbound

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models cites this paper.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary

Reference 262

Resolution
metadata mismatch
local_arxiv, observed 2026-05-21T02:13:55.462937Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:130992f7fb117a16b9877ff7491c0d81e6b8c3a2f32b40110dab778868ecbd1e

Observation 55e7a746-9ee3-4277-9e22-3dc25bb3671e · inbound

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins cites this paper.

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary

Reference 240

Resolution
unresolved
no resolver link, observed 2026-07-11T06:51:42.465920Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:51:42.465920Z digest=sha256:7b521b235e2ad7d2ef3f57292818fcbfd0944e554b6e044a49da23cec20f3422